Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation

Details Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation Lenticular vs spiral galaxies: dark matter content and the Tully-Fisher relation

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15...82b&link_type=abstract

Highlights of Astronomy, Volume 15, p. 82-82

Astronomy and Astrophysics

Astronomy

Scientific paper

We provide observational constraints on disk galaxy evolution for a sample of 28 local edge-on early-type (S0-Sb) disk galaxies. We do this in two ways: (i) we use simple dynamical modelling techniques to constrain their stellar and dark matter content (Williams et al. 2009) and (ii) we compare the zero points of the Tully-Fisher relations (TFRs; Tully & Fisher 1977) of the spirals and S0s.

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